Document Type

Article

Publication Date

5-31-2018

Publication Title

Journal of Geophysical Research

Volume

123

Issue

6

First page number:

1525

Last page number:

1540

Abstract

The recent discovery of some ancient evolved rocks in Gale crater by the Curiosity rover has prompted the hypothesis that continental crust formed in early Martian history. Here we present petrological modeling that attempts to explain this lithological diversity by magma fractionation. Using the thermodynamical software MELTS, we model fractional crystallization of different Martian starting compositions that might generate felsic igneous compositions like those analyzed at Gale crater using different variables, such as pressure, oxygen fugacities, and water content. We show that similar chemical and mineralogical compositions observed in Gale crater felsic rocks can readily be obtained through different degrees of fractional crystallization of basaltic compositions measured on the Martian surface. The results suggest that Gale crater rocks may not represent true liquids as they possibly accumulated and/or fractionated feldspars as well as other phases. In terms of major element compositions and mineralogy, we found that the Gale crater felsic compositions are more similar to fractionated magmas produced in Earth's intraplate volcanoes than to terrestrial felsic continental crust as represented by tonalite-trondhjemite-granodiorite suites. We conclude that the felsic rocks in Gale crater do not represent continental crust, as it is defined on Earth. ©2018. American Geophysical Union. All Rights Reserved.

Keywords

Continental crust; Felsic magmas; Fractional crystallization; Gale crater; Intraplate volcanoes; Mars

Disciplines

Atmospheric Sciences | Geology

File Format

application/pdf

File Size

4.031 Kb

Language

English

Publisher Citation

Udry, A., Gazel, E., & McSween, H. Y., Jr. (2018). Formation of evolved rocks at Gale crater by crystal fractionation and implications for Mars crustal composition. Journal of Geophysical Research: Planets, 123, 1525–1540. https://doi.org/10.1029/2018JE005602

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